Next: Parameter estimation Up: Basic principles of Previous: Time domain analysis . A simple way to graphically present the results of a TSA is to plot the test statistics S against its parameter or l , depending on whether the analysis was performed in the frequency or time domain. ... Examples of statistics used in the time domain are covariance and correlation functions. The correlation of a signal with itself or with another signal produces maxima in these functions at particular lags. ...

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• Corrections to the probability distribution
• Test statistics
• Time series analysis in the frequency domain

... Posts tagged ?posterior distribution? ... stat.AP:0811.1663] . Open Statistical Issues in Particle Physics by Louis Lyons . ... Category: arXiv , Bayesian , Cross-Cultural , Data Processing , Frequentist , High-Energy , Methods , Physics , Stat | ... Accounting for Spatial Correlation in the Scan Statistic by Loh &Zhu [stat.AP:0712.1458] provides a picture that helps us to understand excessive false alarms in source detection when the image data set is based on the Poisson point process. ...

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• Statistics 310 2005-2006
• The AstroStat Slog spatial statistics
• The AstroStat Slog Pareto distribution

... The fitting package in STSDAS (Space Telescope Science Data Analysis System) relies on two basic techniques (one linear and one non-linear) for fitting functions to data. ... Results show that both methods may generate biased coefficients (at the ~few percent level), and over or under-estimate error bars (at the ~10 percent level), in particular from low signal-to-noise data. ... Function coefficient errors are computed directly from the covariance matrix. ... Abscissa is signal-to-noise. ...

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• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• Spatial Models and Spatial Statistics for Astronomical Data
• Heuristic Estimates of Weighted Binomial Statistics for Use in Detecting Rare

... Chapter 14. ... Data consist of numbers, of course. ... In the following sections, you will repeatedly encounter the following paradigm: § apply some formula to the data to compute a statistic § compute where the value of that statistic falls in a probability distribution that is computed on the basis of some null hypothesis § if it falls in a very unlikely spot, way out on a tail of the distribution , conclude that the null hypothesis is false for your ... 603 604 Chapter 14. ...

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• http://www.arcetri.astro.it/irlab/doc/library/recipes/bookcpdf/c14-0.pdf

... The procedure of radiometer signal integration can be considered as a sort of reducing dimension of the initial sampling space, where the samples are the result of analog-to-digital conversion. ... The probability distribution of the signal and spikes is completely known. ... The quality of the considered algorithm could be also illustrated by Figure 2 . ... One could see the considered adaptive algorithm is preferable even by low degree of compression, because all spikes have been depressed. ...

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• Spectral energy distribution

... use frames summary class fields routine details file attributes . ... AUTHOR: Craig B. Markwardt, NASA/GSFC Code 662, Greenbelt, MD 20770 craigm@lheamail.gsfc.nasa.gov UPDATED VERSIONs can be found on my WEB PAGE: http://cow.physics.wisc.edu/~craigm/idl/idl.html . PURPOSE: Compute confidence limits for chi-square statistic . ... CALLING SEQUENCE: DELCHI = MPCHILIM(PROB, DOF, [/SIGMA, /CLEVEL, /SLEVEL ]) . ... result = mpchilim( p , dof , sigma= sigma , clevel= clevel , slevel= slevel ) . ...

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• Bayesian Paradigm
• GLSFit.pro (JWST Pipeline routines in IDL)
• Roelof's Presentations

Andrea Zoia CEA/Saclay DEN/DANS/DM2S/SERMA/LTSD Residence time and collision number statistics : a Feynman-Kac approach International Conference Random Processes, Conformal Field Theory and Integrable Systems September 19 - 23, 2011 Poncelet Laboratory, Moscow, Russia Outline Introduction Stochastic transport : random flights Collision number statistics and diffusion limit Exponential flights and residence ...

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... The observed mean bow is 6.8 \Sigma 1.6 Їrad (1.4 \Sigma0:3 arcsec). ... ISVR current error type value type value Tx 2 ffi's 0.3 mm square \Sigma0.4 mm FW (1) Ty 2 ffi's 1.0 mm square \Sigma1.0 mm FW Tz 2 ffi's 30 \ Theta 10 \Gamma3 mm --- --- --- Rx 2 ffi's 5:0 \ Theta 10 \Gamma5 rad --- --- --- Ry 2 ffi's 5:0 \ Theta 10 \Gamma6 rad --- --- --- Ry 2 ffi's 1:0 \ Theta 10 \Gamma2 rad square \Sigma1:0 \ Theta 10 \Gamma2 rad FW bosses --- --- square \Sigma1:2 \ ...

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• Null-hypothesis probability distribution for a weighted sum of Poissonian
• Intrinsic dispersion
• `Degrees of freedom' for a sum of likelihoods

... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... The Hб  I Column Density Distribution Function at z =0: the Connection to Damped Ly Statistics . ... We present a measurement of the Hб  I column density distribution function [ ] at the present epoch for column densities . These high column densities compare to those measured in damped Ly lines seen in absorption against background quasars. ... The Column Density Distribution Function . ...

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• Pulsar Group Main/Psrfits
• PPTA Wiki | Projects / RedGW
• correlator:distribution [ATNF VLBI Wiki]

Following are instructions to build and install the programs in this distribution. Make sure that you have all necessary tools for building executables. ... The automatic build process expects a configuration file called Config.local . ... The configuration file specifies the directory in which to install the binaries, as well as control over the generation of debugging code and reference clock support. ... Cleans out object files, programs and temporary files. make distclean . ...

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• Monitoring Options
• The Network Time Protocol (NTP) Distribution
• Stats

... The GW from coalescing compact binaries composed of NS and BH are the best understood of all astrophysical GW sources. A conservative lower limit to the event rate of galactic binary neutron star coalescence of about 1 per 100000 year follows from double pulsar   statistics studies (Narayan et al. ... In Figure  47 we show the rates of coalescence of binary WD and NS in a model elliptical galaxy   consisting of stars, depending on time elapsed since the (assumed instantaneous) star formation. ...

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• Dependence on the Scenario Parameters and Initial Distributions
• Frequency distribution of galactic binaries
• Effect of sources evolution on

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• http://zebu.uoregon.edu/~uochep/talks/talks05/G050216-00.pdf
• http://zebu.uoregon.edu/2004/es399/lec05.html
• http://zebu.uoregon.edu/2004/es399/chitable.html

... Public . ... Science Users Information > Science Publications > Science Announcements . ... Public Surveys . ... Published: 24 Feb 2014 . ... The Public ESO Spectroscopic Survey of Transient Objects ( PESSTO ) is one of the two on-going ESO public spectroscopic surveys . ... The first public data release ( DR1 ) of the VIDEO programme via the ESO Science Archive Facility, contained 97 individual (i.e. single-OB) tile images in the VIDEO-XMM3 field and their associated single-band source lists. ...

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• ESO - Newsletter October 2015
• Documentation
• Redshift Distribution

... According to the most popular cosmological paradigm, the greater part of the galaxy mass is accumulated in the dark matter halo. ... The polar ring galaxies (PRGs) reveal external rings or disks of gas, dust and stars rotating in a plane roughly perpendicular to the disk of the central galaxy. ... The shape of the dark halo in the model was chosen so as to achieve the best fit to the observed rotation of both galaxies themselves and their polar rings. ... The SPRC-7 galaxy. ...

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Next: Data reduction: moments Up: No Title Previous: Feature enhancement: local . ... When this is done for the energy map, with the energy scale distributed logarithmically, the result is shown on Fig. ... It can be shown that the mean magnitude at each duration reproduces the mean power spectrum in log-log coordinates. Therefore, this particular presentation of the probability density function shows graphically the scale-dependent scatter around the mean energy spectrum. ...

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• Historical Notes
• Energy distribution
• Pyramidal (multiresolution) true-rectangular TF tiling

... The absolute magnitude of the RCBs in the LMC and the small number of Galactic RCBs implies that they are very rare stars. Together with statistics for related stars, the total number of hydrogen-deficient stars in the Galaxy is estimated to be about 1000. Whilst the luminosity of RCBs is similar to that of other low-mass stars as they evolve rapidly from the asymptotic RED GIANT branch to become WHITE DWARFS , their frequency is much lower. ...

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• Galactic distribution and absolute magnitudes
• C. Refereed Journal Publications 2001
• Irregular Satellite Research

... Results 3. ... 2004), Escapa (2011): Hamiltonian approach, simplified elastic response. ... PАg. ... Let us recall that assuming a rheological model based in Smith (1974) , Wahr (1979) and IERS (2010) for the elastic/anelastic response of the Earth, the second order harmonic components of the redistribution potential admit a truncated development in complex spherical harmonics in the form Generalized Love Numbers, dependent on: Harmonic order, Excitation frequencies In magnitude, PАg. ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/kudryashova.pdf
• http://www.gao.spb.ru/english/as/publ/gorshkov_geocosmos-2014.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/gorshkov2.pdf

... Chubukova I. - Data Mining (2007) PDF Data Mining . Hand D. Mannila H. Smyth P. - Principles of data mining (2001) DJVU Data Mining . Mitra S. Acharya T. - Data mining (2003) (In Russian) DJVU Data Mining . Abbass H. Sarker R. Newton C. - Data Mining Heuristic Approach (2002) PDF Data Mining . Rao C. Wegman E. Solka J. - Handbook of Statistics Data Mining and Data Visualization (2004) PDF Data Mining . ... Whittet D. - Dust in galaxies (2003) PDF Межзвездная среда . ...

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These lesson introduces you to the use of uncertainties. In particular how to interpret them, and how to factor them in when working out if a theory or prediction is good. It introduces probability distribution functions, the Gaussian Distribution, hypothesis testing and model fitting. Back Main Uncertainties Page .

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• Lab Skills Video Tutorials: Uncertainties
• Siding Spring Survey
• The GMRT Array Distribution

Magnetic Fields around Radio Galaxies Robert Laing (ESO) Laing et al. ... 2008) Negligible depolarization and 2 rotation Almost all Faraday effects must be due to foreground material How to fit depolarization caused by foreground Faraday rotation Complex polarization Rotation measure Integrate over a beam Observed RM for 0 2 rotation and depolarization Faraday rotation and depolarization 5.5 arcsec FWHM Faraday effects at high resolution FWHM = 1.5 ...

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• http://www.mrao.cam.ac.uk/~anthony/latex/McKean.ps
• http://www.mrao.cam.ac.uk/~bn204/lecture/2008/bn-l1.pdf
• http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/AHall-P.pdf